Meteor, also called a shooting star, or falling star, streak of light
in the sky that results when a particle or small chunk of stony or
metallic matter enters the Earth's atmosphere and vaporizes. The term
is sometimes applied to the falling object itself, but the latter is
properly called a meteoroid. The vast majority of meteoroids
burn up in the upper atmosphere, but occasionally one of relatively
large mass survives its fiery plunge and reaches the surface as a
solid body. Such an object is known as a meteorite.

The speed at which a meteoroid enters the upper atmosphere is
dependent primarily on two motions--that of the meteoroid in its
elongated orbit and that of the Earth in its path around the Sun.
Also, the Earth's gravitational pull on the meteoroid increases its
velocity by 3 km (1.9 miles) per second or more. Observations have
shown that meteoroids penetrate the atmosphere at velocities ranging
from 11 to 72 km (7 to 45 miles) per second.

When a meteoroid plunges toward the Earth at high speed, its surface
collides with the atoms and molecules of the atmosphere. These
collisions dislodge material from the meteoroid's surface and break
up atoms and molecules of both the meteoroid and atmosphere into
charged particles. The ionized atoms are excited to produce visible
light. Much of this light is generated near the moving solid body,
but in the case of very fast, bright meteors a residual luminosity
called the train may be left behind the meteor head. As the meteoroid
plunges closer to the ground, an extremely dense, hot gas cap
develops in front of it. A shock wave also may be produced in the air
ahead of the meteoroid. Such atmospheric shock waves may propagate to
the Earth's surface because meteoroids travel through the air at five
times the speed of sound or higher. A meteoroid weighing about 1 kg
(2.2 pounds) penetrating to an altitude of roughly 40 km (25 miles)
can produce sounds on the ground resembling thunder or sonic booms.

Most meteoroids crumble and disintegrate completely before they reach
an altitude of 80 km (50 miles). It has been speculated that
meteoroids that readily fragment originated with comets, whereas the
denser objects that penetrate to the surface are remnants of
asteroids that broke apart hundreds of millions of years ago.

When the Earth encounters swarms of meteoroids moving together,
meteor showers become visible. Photographic data indicate that many
such phenomena are associated with the orbits of observed comets. For
example, the meteor shower known as Eta Aquarid, which can be seen
each year in early May, has been identified with Halley's Comet. The
meteoroids in the swarm producing this shower are thought to be
debris ejected from the comet along its orbit.

Much accurate observational data on meteors has been obtained in
recent years by means of special high-speed, wide-angle cameras and
electronic image intensifiers. Radar also has been widely used in
studying meteors, since radio waves can be bounced off the ionized
gases yielded by the vaporizing constituent matter. It is very useful
in determining the speed, direction, and height of meteors,
particularly in daylight and under weather conditions unfavourable
for visual observations.